Distance from Earth: 346.1 parsecs (1,129.0 light years)
The transit method detects planets by measuring the periodic dimming of a star's brightness as a planet passes in front of it. NASA's Kepler and TESS missions have used this technique to discover the majority of known exoplanets. The depth of the brightness dip reveals the planet's size relative to its star, while the period between transits gives the orbital period.
Radius
9.10 R⊕
57,987 km
Mass
8,899.20 M⊕
5.31E28 kg
Orbital Period
5.38 days
0.015 years
Eq. Temperature
1369 K
1096°C
Orbital Semi-major Axis
0.0619 AU
Density
65.80 g/cm³
9.10x Earth
8,899.20x Earth
0.015x Earth
Star Temperature
5,820 K
Star Radius
1.47 R☉
Star Mass
1.07 M☉
Planets in System
1
Stars in System
1
1369 K is outside the range for liquid water (180-310 K).
9.10 Earth radii suggests a non-rocky composition.
Receives 580.00x Earth's insolation, outside the habitable zone.
This planet orbits outside the estimated habitable zone of its star.
Habitability assessments are rough estimates based on limited available data. True habitability depends on many additional factors including atmospheric composition, magnetic field presence, tidal locking, and stellar activity. These assessments should not be considered definitive.
Eccentricity
0.0940
Insolation Flux
580.00 S⊕
Earth flux = 1.0
4.75x Earth